THE TIME DISTRIBUTION OF EAS WITH E>1014eV

  • We have observed the arrival times of EAS initiated by cosmic rays of E>1014eV using the EAS array in Beijing. The distribution of arrival time intervals of EAS With E>2.6×1014eV is considerably higher than the exponential distribution in the region of time interval t<21 second. It is suggested that a time correlation component is probably present in the EAS events.
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  • [1] M. Grewing, et al., Astrophys. Lett., S(1971 ), 167.[2] J. A. Murphy et al., 16th ICRC, 1(1979), 248.P. N. Bhat et al., 16th ICRC, 1(1979), 216.李惕暗, 自然, INo. 8(1978),469.[3] B. Mcbreen et al., 17th ICRC, 6(1981), 301.[4] V. P. Fomin et al., 17th ICRC, 1(1981), 28.[5] J. B. Mukanov et al., Astrof. Abs., 62(1980), 98.[6] S. Danaher et al., Nature 28 (1981), 568.[7] C. IvIorello et al., 18th ICRC, 1(1983j, 127.[8] W. Stamm et al., 18th ICRC, 1(1983), 131.[9] C. L. Bhat et al., 16th ICRC, 8(1979), 57.[10] D. J. Fegan et al., 17th ICRC, 6(1981), 296.[11] 陈映宣等, 高能物理与核物理, 4(1980),683,[12] 王立祥, 高能物理研究所宇宙线研究室年报, 1981-1982, P, 50,[13] 何长孝等, 郑州大学学报(自然科学版),1983年增刊, P. 0_03.[14] 李惕陪, 实验的数学处理, 科学出版社, 1980年2月第一版.[15] 何长孝等, 高能宇宙线粒子时间分布实验数据的进一步分析和模拟, 高能物理研究所宇线研究室年报, 1983 P.79,
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CHEN Ying-Xuan, HE Chang-Xiao, XIAO Qian-Yi and WANG Li-Xiang. THE TIME DISTRIBUTION OF EAS WITH E>1014eV[J]. Chinese Physics C, 1985, 9(4): 391-396.
CHEN Ying-Xuan, HE Chang-Xiao, XIAO Qian-Yi and WANG Li-Xiang. THE TIME DISTRIBUTION OF EAS WITH E>1014eV[J]. Chinese Physics C, 1985, 9(4): 391-396. shu
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Received: 1900-01-01
Revised: 1900-01-01
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THE TIME DISTRIBUTION OF EAS WITH E>1014eV

    Corresponding author: CHEN Ying-Xuan,

Abstract: We have observed the arrival times of EAS initiated by cosmic rays of E>1014eV using the EAS array in Beijing. The distribution of arrival time intervals of EAS With E>2.6×1014eV is considerably higher than the exponential distribution in the region of time interval t<21 second. It is suggested that a time correlation component is probably present in the EAS events.

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